Galaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm

Driver, SimonRobotham, A. S. G.Kelvin, L SAlpaslan, MBaldry, I. K.Bamford, Steven P.Brough, SarahBrown, MHopkins, Andrew M.Liske, JochenColless, MatthewMadore, BarrySharp, RobertTuffs, Richard Jvan Kampen, EAndrae, Ellen2015-12-130035-8711http://hdl.handle.net/1885/78393We use the Galaxy And Mass Assembly survey (GAMA) I data set combined with GALEX, Sloan Digital Sky Survey (SDSS) and UKIRT Infrared Deep Sky Survey (UKIDSS) imaging to construct the low-redshift (z < 0.1) galaxy luminosity functions in FUV, NUV, ugrizAuthor/s retain copyrightKeywords: Fundamental parameters-galaxies; Galaxies; General-galaxies; Luminosity function, mass function-cosmology; Observations-infrared; Surveys-galaxiesGalaxy And Mass Assembly (GAMA): The 0.013 < z < 0.1 cosmic spectral energy distribution from 0.1 m to 1 mm201210.1111/j.1365-2966.2012.220362016-02-24